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Some aspects of stochastic differential equations driven by - - PowerPoint PPT Presentation

Some aspects of stochastic differential equations driven by fractional Brownian motions Fabrice Baudoin Purdue University Based on joint works with L. Coutin, M. Hairer, C. Ouyang and S. Tindel Motivation The motivation of the talk is to


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Some aspects of stochastic differential equations driven by fractional Brownian motions

Fabrice Baudoin

Purdue University

Based on joint works with L. Coutin, M. Hairer, C. Ouyang and

  • S. Tindel
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Motivation

The motivation of the talk is to present some results concerning solutions of stochastic differential equations on Rn X x

t = x +

t V0(X x

s )ds + d

  • i=1

t Vi(X x

s )dBi s

(1) where the Vi’s are C ∞-bounded vector fields on Rn and B is a d-dimensional fractional Brownian motion.

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Motivation

The motivation of the talk is to present some results concerning solutions of stochastic differential equations on Rn X x

t = x +

t V0(X x

s )ds + d

  • i=1

t Vi(X x

s )dBi s

(1) where the Vi’s are C ∞-bounded vector fields on Rn and B is a d-dimensional fractional Brownian motion. More precisely, we shall be interested in the properties of the distribution of X x

t :

Existence of a smooth density;

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Motivation

The motivation of the talk is to present some results concerning solutions of stochastic differential equations on Rn X x

t = x +

t V0(X x

s )ds + d

  • i=1

t Vi(X x

s )dBi s

(1) where the Vi’s are C ∞-bounded vector fields on Rn and B is a d-dimensional fractional Brownian motion. More precisely, we shall be interested in the properties of the distribution of X x

t :

Existence of a smooth density; Small-time asymptotics;

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Motivation

The motivation of the talk is to present some results concerning solutions of stochastic differential equations on Rn X x

t = x +

t V0(X x

s )ds + d

  • i=1

t Vi(X x

s )dBi s

(1) where the Vi’s are C ∞-bounded vector fields on Rn and B is a d-dimensional fractional Brownian motion. More precisely, we shall be interested in the properties of the distribution of X x

t :

Existence of a smooth density; Small-time asymptotics; Smoothing properties of the operator Ptf (x) = E(f (X x

t ));

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Motivation

The motivation of the talk is to present some results concerning solutions of stochastic differential equations on Rn X x

t = x +

t V0(X x

s )ds + d

  • i=1

t Vi(X x

s )dBi s

(1) where the Vi’s are C ∞-bounded vector fields on Rn and B is a d-dimensional fractional Brownian motion. More precisely, we shall be interested in the properties of the distribution of X x

t :

Existence of a smooth density; Small-time asymptotics; Smoothing properties of the operator Ptf (x) = E(f (X x

t ));

Functional inequalities satisfied by the law of the solution and upper Gaussian bounds for the density.

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Fractional Brownian motion

A fractional Brownian motion is a Gaussian process with mean 0 and covariance function 1 2

  • t2H + s2H + |t − s|2H

.

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Fractional Brownian motion

A fractional Brownian motion is a Gaussian process with mean 0 and covariance function 1 2

  • t2H + s2H + |t − s|2H

. Stochastic differential equations driven by fractional Brownian motions provide toy models for the study of non Markov random dynamical systems.

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Fractional Brownian motion

A fractional Brownian motion is a Gaussian process with mean 0 and covariance function 1 2

  • t2H + s2H + |t − s|2H

. Stochastic differential equations driven by fractional Brownian motions provide toy models for the study of non Markov random dynamical systems. Let H > 1/2. The equation is understood in the Young’s sense.

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Fractional Brownian motion

A fractional Brownian motion is a Gaussian process with mean 0 and covariance function 1 2

  • t2H + s2H + |t − s|2H

. Stochastic differential equations driven by fractional Brownian motions provide toy models for the study of non Markov random dynamical systems. Let H > 1/2. The equation is understood in the Young’s sense. Existence and uniqueness of the solution of (1) have been discussed by Nualart-Rascanu and Zähle.

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Fractional Brownian motion

A fractional Brownian motion is a Gaussian process with mean 0 and covariance function 1 2

  • t2H + s2H + |t − s|2H

. Stochastic differential equations driven by fractional Brownian motions provide toy models for the study of non Markov random dynamical systems. Let H > 1/2. The equation is understood in the Young’s sense. Existence and uniqueness of the solution of (1) have been discussed by Nualart-Rascanu and Zähle. Let H > 1/4. The equation is understood in the Lyons’ rough paths sense.

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Fractional Brownian motion

A fractional Brownian motion is a Gaussian process with mean 0 and covariance function 1 2

  • t2H + s2H + |t − s|2H

. Stochastic differential equations driven by fractional Brownian motions provide toy models for the study of non Markov random dynamical systems. Let H > 1/2. The equation is understood in the Young’s sense. Existence and uniqueness of the solution of (1) have been discussed by Nualart-Rascanu and Zähle. Let H > 1/4. The equation is understood in the Lyons’ rough paths sense. See Coutin-Qian.

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Hörmander’s type theorem

Let H > 1/2.

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Hörmander’s type theorem

Let H > 1/2. If I = (i1, . . . , ik) ∈ {0, . . . , d}k, we denote by VI the Lie commutator defined by VI = [Vi1, [Vi2, . . . , [Vik−1, Vik] . . .] and d(I) = k + n(I), where n(I) is the number of 0 in the word I. Theorem (Baudoin-Hairer, PTRF’07) Assume that, at some x0 ∈ Rn, there exists N such that: span{VI(x0), d(I) ≤ N} = Rn.

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Hörmander’s type theorem

Let H > 1/2. If I = (i1, . . . , ik) ∈ {0, . . . , d}k, we denote by VI the Lie commutator defined by VI = [Vi1, [Vi2, . . . , [Vik−1, Vik] . . .] and d(I) = k + n(I), where n(I) is the number of 0 in the word I. Theorem (Baudoin-Hairer, PTRF’07) Assume that, at some x0 ∈ Rn, there exists N such that: span{VI(x0), d(I) ≤ N} = Rn. (2) Then, for any t > 0, the law of the random variable X x0

t

has a smooth density with respect to the Lebesgue measure on Rn.

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Scheme of the proof

Since Malliavin (76), the scheme of the proof is quite standard but here, it requires new estimation methods since we are in a non-semimartingale setting.

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Scheme of the proof

Since Malliavin (76), the scheme of the proof is quite standard but here, it requires new estimation methods since we are in a non-semimartingale setting. The main difficulty is to prove a Norris type lemma for stochastic integrals with respect to fBm.

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Scheme of the proof

Since Malliavin (76), the scheme of the proof is quite standard but here, it requires new estimation methods since we are in a non-semimartingale setting. The main difficulty is to prove a Norris type lemma for stochastic integrals with respect to fBm.

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Scheme of the proof

Since Malliavin (76), the scheme of the proof is quite standard but here, it requires new estimation methods since we are in a non-semimartingale setting. The main difficulty is to prove a Norris type lemma for stochastic integrals with respect to fBm. Computation of the Malliavin matrix.

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Scheme of the proof

Since Malliavin (76), the scheme of the proof is quite standard but here, it requires new estimation methods since we are in a non-semimartingale setting. The main difficulty is to prove a Norris type lemma for stochastic integrals with respect to fBm. Computation of the Malliavin matrix. Proof of its invertibility and Lp estimates on its inverse.

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Scheme of the proof

Since Malliavin (76), the scheme of the proof is quite standard but here, it requires new estimation methods since we are in a non-semimartingale setting. The main difficulty is to prove a Norris type lemma for stochastic integrals with respect to fBm. Computation of the Malliavin matrix. Proof of its invertibility and Lp estimates on its inverse.

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Recent developments

Existence of the density H > 1/4 by Cass-Friz (2010),

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Recent developments

Existence of the density H > 1/4 by Cass-Friz (2010), Smoothness with H > 1/3 in some particular cases by Hu-Tindel (2011)

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Recent developments

Existence of the density H > 1/4 by Cass-Friz (2010), Smoothness with H > 1/3 in some particular cases by Hu-Tindel (2011) Smoothness with H > 1/3 in the general case by Hairer-Pillai (2011) + Cass-Litterer-Lyons (2011).

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Operators associated with SDEs driven by fBms

Again, let us consider the stochastic differential equations on Rn X x0

t

= x0 +

d

  • i=1

t Vi(X x0

s )dBi s

(3) where the Vi’s are C ∞-bounded vector fields on Rn and B is a d dimensional fractional Brownian motion with Hurst parameter H > 1

3.

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Operators associated with SDEs driven by fBms

Again, let us consider the stochastic differential equations on Rn X x0

t

= x0 +

d

  • i=1

t Vi(X x0

s )dBi s

(3) where the Vi’s are C ∞-bounded vector fields on Rn and B is a d dimensional fractional Brownian motion with Hurst parameter H > 1

3.

We denote by C∞

b (Rn, R) the set of compactly supported smooth

functions Rn → R. If f ∈ C∞

b (Rn, R), let us denote

Ptf (x0) = E (f (X x0

t )) , t ≥ 0,

where X x0

t

is the solution of (3) at time t.

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Development in small times

Theorem (Baudoin-Coutin, SPA’07) Assume H > 1

  • 3. There exists a family
  • ΓH

k

  • k≥0 of differential
  • perators such that:

If f ∈ C∞

b (Rn, R) and x ∈ Rn, then for every N ≥ 0, when t → 0

Ptf (x) =

N

  • k=0

t2kH(ΓH

k f )(x) + o(t(2N+1)H).

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Development in small times

1

ΓH

1 = 1

2

d

  • i=1

V 2

i ;

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Development in small times

1

ΓH

1 = 1

2

d

  • i=1

V 2

i ;

2

ΓH

2 = H

4 β(2H, 2H)

d

  • i,j=1

V 2

i V 2 j +

2H − 1 8(4H − 1)

d

  • i,j=1

ViV 2

j Vi

+

  • H

4(4H − 1) − H 4 β(2H, 2H)

  • d
  • i,j=1

(ViVj)2, where β(a, b) = 1

0 xa−1(1 − x)b−1dx;

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Development in small times

1

ΓH

1 = 1

2

d

  • i=1

V 2

i ;

2

ΓH

2 = H

4 β(2H, 2H)

d

  • i,j=1

V 2

i V 2 j +

2H − 1 8(4H − 1)

d

  • i,j=1

ViV 2

j Vi

+

  • H

4(4H − 1) − H 4 β(2H, 2H)

  • d
  • i,j=1

(ViVj)2, where β(a, b) = 1

0 xa−1(1 − x)b−1dx;

3 More generally, ΓH

k is a homogeneous polynomial in the V ′ i s of

degree 2k: ΓH

k =

  • I=(i1,...i2k)

aIVi1...Vi2k,

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Development in small times

We conjecture that ΓH

k , k ≥ 2, has coefficients that are

meromorphic functions of H with poles in the set { 1

2j , 2 ≤ j ≤ k}.

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Development in small times

We conjecture that ΓH

k , k ≥ 2, has coefficients that are

meromorphic functions of H with poles in the set { 1

2j , 2 ≤ j ≤ k}.

It would be interesting to determine what is the smallest algebra of vector fields that contains the family (ΓH

k )k≥1 ( In

the case of Brownian motion, this algebra is the algebra generated by the operator d

i=1 V 2 i ).

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Smoothing property

As already seen, under the ellipticity assumption span {V1(x), · · · , Vn(x)} = Rn,

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Smoothing property

As already seen, under the ellipticity assumption span {V1(x), · · · , Vn(x)} = Rn, the functional operator Ptf (x) = E (f (X x

t ))

has a smooth integral kernel.

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Smoothing property

As already seen, under the ellipticity assumption span {V1(x), · · · , Vn(x)} = Rn, the functional operator Ptf (x) = E (f (X x

t ))

has a smooth integral kernel. We prove here the following regularisation bounds, for q > 1, |Vi1 · · · VikPtf (x)| ≤ Ck,q(x) tkH (Pt|f |q)1/q (x), 0 < t < 1.

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Smoothing property

As already seen, under the ellipticity assumption span {V1(x), · · · , Vn(x)} = Rn, the functional operator Ptf (x) = E (f (X x

t ))

has a smooth integral kernel. We prove here the following regularisation bounds, for q > 1, |Vi1 · · · VikPtf (x)| ≤ Ck,q(x) tkH (Pt|f |q)1/q (x), 0 < t < 1. which implies |Vi1 · · · VikPtf (x)| ≤ Ck(x) tkH f ∞, 0 < t < 1.

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Integration by parts on the path space

The keypoint is to use integration by parts formulas obtained through Malliavin calculus.

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Integration by parts on the path space

The keypoint is to use integration by parts formulas obtained through Malliavin calculus. Since we assume ellipticity [Vi, Vj] =

n

  • k=1

ωk

ijVk.

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Integration by parts on the path space

The keypoint is to use integration by parts formulas obtained through Malliavin calculus. Since we assume ellipticity [Vi, Vj] =

n

  • k=1

ωk

ijVk.

We first have the following commutation Lemma ViPtf (x) = E n

  • k=1

αk

i (t, x)Vkf (X x t )

  • ,

where α solves the following system of SDEs: dαj

i(t, x) = n

  • k,l=1

αk

i (t, x)ωj kl(X x t )dBl t,

αj

i(0, x) = δj i .

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Integration by parts on the path space

Proof. By the chain rule ViPtf (x) =

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Integration by parts on the path space

Proof. By the chain rule ViPtf (x) = E ((JtVi)f (X x

t ))

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Integration by parts on the path space

Proof. By the chain rule ViPtf (x) = E ((JtVi)f (X x

t )) = E ((Φt∗Vi)f (X x t )) .

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Integration by parts on the path space

Proof. By the chain rule ViPtf (x) = E ((JtVi)f (X x

t )) = E ((Φt∗Vi)f (X x t )) .

Then by ellipticity, we can find αj

i(t, x) such that

Φt∗Vi(X x

t ) = n

  • j=1

αj

i(t, x)Vj(X x t ).

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Integration by parts on the path space

Proof. By the chain rule ViPtf (x) = E ((JtVi)f (X x

t )) = E ((Φt∗Vi)f (X x t )) .

Then by ellipticity, we can find αj

i(t, x) such that

Φt∗Vi(X x

t ) = n

  • j=1

αj

i(t, x)Vj(X x t ).

The change of variable formula shows that α solves the above system of SDEs.

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Integration by parts on the path space

We introduce the following scale of spaces:

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Integration by parts on the path space

We introduce the following scale of spaces: Definition For r ∈ R, let Kr be the set of mapping Φ : (0, 1] × Rn → D∞ such that:

1 Almost surely, Φ(t, x) is smooth with respect to x and ∂Φ

∂xν is

continuous in (t, x).

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Integration by parts on the path space

We introduce the following scale of spaces: Definition For r ∈ R, let Kr be the set of mapping Φ : (0, 1] × Rn → D∞ such that:

1 Almost surely, Φ(t, x) is smooth with respect to x and ∂Φ

∂xν is

continuous in (t, x).

2 For every n, p > 1,

sup

0<t≤1

t−rH

  • ∂Φ

∂xν

  • Dk,p < ∞
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Integration by parts on the path space

We introduce the following scale of spaces: Definition For r ∈ R, let Kr be the set of mapping Φ : (0, 1] × Rn → D∞ such that:

1 Almost surely, Φ(t, x) is smooth with respect to x and ∂Φ

∂xν is

continuous in (t, x).

2 For every n, p > 1,

sup

0<t≤1

t−rH

  • ∂Φ

∂xν

  • Dk,p < ∞
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Integration by parts on the path space

The key step is then the following integration by parts on the path space of fBm.

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Integration by parts on the path space

The key step is then the following integration by parts on the path space of fBm. Theorem If f is C ∞-bounded and Φ ∈ Kr, E (Φ(t, x)Vif (X x

t )) = E ((TViΦ)(t, x)f (X x t ))

for some TViΦ ∈ Kr−1.

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Integration by parts on the path space

Dj

sf (Xt) = ∇f (Xt), Dj sX x t

= ∇f (Xt), JtJ−1

s Vj(X x s )

=

n

  • k,l=1

hj

k(s, t, x)αk l (t, x)(Vlf )(X x t ).

where hi(s, t, x) = (βk

i (s, x)I[0,t](s))k=1,...,n,

i = 1, ..., n.

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Integration by parts on the path space

Dj

sf (Xt) = ∇f (Xt), Dj sX x t

= ∇f (Xt), JtJ−1

s Vj(X x s )

=

n

  • k,l=1

hj

k(s, t, x)αk l (t, x)(Vlf )(X x t ).

where hi(s, t, x) = (βk

i (s, x)I[0,t](s))k=1,...,n,

i = 1, ..., n. Introduce Mi,j(t, x) given by Mi,j(t, x) = 1 t2H hi(·, t, x), hj(·, t, x)H. Hence Vif (X x

t ) =

1 t2H

n

  • j,l=1

βi

j(t, x)M−1 jl (t)Df (X x t ), hl(·, t)H.

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Integration by parts on the path space

Using then the integration by parts formula for the Malliavin derivative, we obtain

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Integration by parts on the path space

Using then the integration by parts formula for the Malliavin derivative, we obtain T ∗

ViΦ(t, x) = n

  • k,l=1

1 t2H Φ(t, x)βi

k(t, x)M−1 kl (t)δhl(·, t)

− 1 t2H D(Φ(t, x)βi

k(t, x)M−1 kl (t)), hl(·, t)H

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Regularizing bounds

Iterating the previous formulas and using Hölder’s inequality, we finally conclude:

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Regularizing bounds

Iterating the previous formulas and using Hölder’s inequality, we finally conclude: Theorem (Baudoin-Ouyang, 2011) For q > 1, |Vi1 · · · VikPtf (x)| ≤ Ck,q(x) tkH (Pt|f |q)1/q (x), 0 < t < 1.

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Global bounds

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Global bounds

In some geometric situations, it is possible to obtain global bounds independent from x.

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Global bounds

In some geometric situations, it is possible to obtain global bounds independent from x. Assume the skew-symmetry condition ωk

ij = −ωj ik,

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Global bounds

In some geometric situations, it is possible to obtain global bounds independent from x. Assume the skew-symmetry condition ωk

ij = −ωj ik,

then we have the global bound

  • n
  • i=1

(ViPtf )2(x) ≤ Pt  

  • n
  • i=1

(Vif )2   (x).

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Global bounds

In a recent work with C. Ouyang and S. Tindel, we proved that under the same structure assumptions, we have the Gaussian concentration

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Global bounds

In a recent work with C. Ouyang and S. Tindel, we proved that under the same structure assumptions, we have the Gaussian concentration Theorem (Baudoin-Ouyang-Tindel, 2011) There exists M such that for every T ≥ 0 and λ ≥ 0, P

  • sup

0≤t≤T

X x

t − E

  • sup

0≤t≤T

X x

t

  • ≥ λ
  • ≤ exp

λ2 2MT 2H

  • .
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Global bounds

In a recent work with C. Ouyang and S. Tindel, we proved that under the same structure assumptions, we have the Gaussian concentration Theorem (Baudoin-Ouyang-Tindel, 2011) There exists M such that for every T ≥ 0 and λ ≥ 0, P

  • sup

0≤t≤T

X x

t − E

  • sup

0≤t≤T

X x

t

  • ≥ λ
  • ≤ exp

λ2 2MT 2H

  • .

and a corresponding Gaussian upper bound.

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Global bounds

Theorem (Baudoin-Ouyang-Tindel, 2011) For any t ∈ R∗

+, the random variable X x t admits a smooth density

pX(t, ·).

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Global bounds

Theorem (Baudoin-Ouyang-Tindel, 2011) For any t ∈ R∗

+, the random variable X x t admits a smooth density

pX(t, ·). Furthermore, there exist 3 positive constants c(1)

t

, c(2)

t

, c(3)

t,x such that

pX(t, y) ≤ c(1)

t

exp

  • −c(2)

t

  • y − c(3)

t,x

2 , for any y ∈ Rd.

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Global bounds

Again, under the structure assumption we also have a global Poincaré inequality:

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Global bounds

Again, under the structure assumption we also have a global Poincaré inequality: Theorem (Baudoin-Ouyang-Tindel, 2011) Pt(f 2) − (Ptf )2 ≤ Ct2HPt n

  • i=1

(Vif )2

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Global bounds

Again, under the structure assumption we also have a global Poincaré inequality: Theorem (Baudoin-Ouyang-Tindel, 2011) Pt(f 2) − (Ptf )2 ≤ Ct2HPt n

  • i=1

(Vif )2

  • a log-Sobolev inequality:

Theorem (Baudoin-Ouyang-Tindel, 2011) Pt(f ln f ) − (Ptf )(ln Ptf ) ≤ 2Ct2HPt n

  • i=1

(Vi ln f )2 f